Statistics – Computation
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.275..109v&link_type=abstract
In ESA, Proceedings of the 21st ESLAB Symposium on Small Scale Plasma Processes in the Solar Chromosphere/Corona, Interplanetary
Statistics
Computation
2
Coronal Loops, Magnetic Field Configurations, Magnetohydrodynamic Stability, Solar Corona, Solar Magnetic Field, Viscosity, Computational Fluid Dynamics, Stress Tensors, Thermomagnetic Effects
Scientific paper
The study of resistive ballooning instabilities in line-tied coronal magnetic fields is extended by including viscosity in the stability analysis. The equations that govern the resistive ballooning instabilities are derived and the effects of viscosity are included using Braginskii's stress tensor. Numerical solutions to the equations are obtained under the rigid wall boundary conditions for arcades with cylindrically symmetric magnetic fields. The stabilizing influences of parallel and perpendicular viscosity are investigated. Perpendicular viscosity is more important and can lead to complete stabilization.
Goossens Marcel
Hood Alan William
Vanderlinden R.
No associations
LandOfFree
The effects of viscosity on resistive ballooning modes in line-tied coronal magnetic fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The effects of viscosity on resistive ballooning modes in line-tied coronal magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effects of viscosity on resistive ballooning modes in line-tied coronal magnetic fields will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1340612